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Geological evidence of Mercury’s chaotic orbit

3 mai 2023

In a study conducted by Paris Observatory - PSL and Sorbonne University, a sedimentary record confirms the strong chaos in the Solar System and the strong instability of the planet Mercury, 117 million years ago. The study is to be published in Earth and Planetary Science Letters, May 15, 2023.

The elliptical orbits of the planets of the Solar System are governed by the laws of universal gravitation and celestial mechanics. Astronomical modeling shows that this results in a chaotic system due to the interactions between the planets of the Solar System and the Sun, with possible instabilities in the planetary orbits.

Le système solaire
© Y. Gominet/IMCCE/NASA

The inner planets (Mercury, Venus, Earth and Mars) are the most concerned by this phenomenon of chaos, given their relatively small masses.

One of the expressions of this system is the highlighting in astronomical models of several resonant terms, that is to say of linear relations between orbital periodicities of the inner planets. Because of the chaos, these orbital cyclicities, present in the resonant terms, undergo variations of their periodicity at the scale of several tens of millions of years (Ma).

For ancient times, beyond about 50 Ma, these resonant terms can only be revealed in sedimentary series that have recorded paleo-environmental variations, themselves induced by changes in insolation at the Earth’s surface governed by the parameters of the Earth’s orbit.

Alternances marnes-calcaires de l’Aptien
(Angles, Alpes de Haute-Provence). Chaque alternance représente un cycle de précession de 20 000 ans.
G. Charbonnier

Through an exceptional sedimentary record of astronomical periodicities of different frequencies on an outcrop of southeastern France dated from the Cretaceous, on the interval 113-123 Ma, the study, led by two laboratories, including the Institute of Celestial Mechanics and Calculation of Ephemerides at the Paris Observatory - PSL, has clearly highlighted a transition to 117 Ma in a resonant term.

Correspondance remarquable entre données géologiques et modèle astronomique
(A) Analyse fréquentielle des variations de susceptibilité magnétique sur la série sédimentaire de l’Aptien dans le sud-est de la France (intervalle 113-122 Millions d’années). A gauche : filtrage à basse fréquence. A droite : spectrogramme d’amplitude évolutif, une transition dans le terme d’excentricité gMercure–gJupiter est enregistrée vers 117.19 Ma. (B) Analyse fréquentielle des variations basse-fréquence de l’excentricité de l’orbite terrestre pour les derniers 180 Ma selon le modèle astronomique La2004. A gauche : filtrage à basse fréquence. A droite : spectrogramme d’amplitude évolutif, une transition, à la fois dans les termes d’excentricité gMercure–gJupiter et gMercure–gVénus, est centrée à 117.2 Ma.

The scientists confirm not only the strong chaos in the inner Solar System, but also the strong instability of the orbit of the planet Mercury.

In parallel, the analysis of the astronomical model La2004, probably the most reliable of all existing models (at least on the long term evolutions), also reveals a concomitant transition centered at 117 Ma in several resonant terms.

Reference
Astrochronology of the Aptian stage and evidence for the chaotic orbital motion of Mercury, Earth and Planetary Science Letters, 15 May 2023.

This result was acquired in the framework of the ANR AstroMeso and ERC AstroGeo projects coordinated by J. Laskar (Observatoire de Paris, IMCCE - UMR 8028).

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